Download Energy Transfer in the Atomosphere

Sci 10 – Unit 4(10.2)
Energy Transfer in the Atmosphere (Notes)
Energy Transfer in the Atmosphere – Notes
What is Earth’s Atmosphere Like?
Many planets have atmospheres, layers of gases that extend above a planet’s surface.
Earth’s atmosphere is made up a five layers: from lowest to highest, they are the
troposphere, stratosphere, mesosphere, thermosphere, and exosphere. These layers
different in chemical composition, average temperature, and density.
The troposphere is the layer nearest the surface of the Earth. Almost all water vapour and
dust in the atmosphere is found here. The average temperature near Earth is 15 o C but at
the top of the troposphere is -55oC. 99% of the gases in the troposphere are nitrogen and
oxygen.
The stratosphere has dry air and an average temperature of about -55oC at the bottom and
0oC at the top. The ozone layer, which absorbs much of the ultraviolet radiation from the
Sun, is in the stratosphere.
Temperatures in the thermosphere can reach 1500 oC to 3000oC. The northern lights, or
aurora borealis, are a result of charged particles colliding in the thermosphere.
The boundaries of the exosphere are not well defined, and this layer merges with outer
space.
The atmosphere is constantly changing, due to many factors, including the Sun’s rotation
and the effects of day and night.
How is the Atmosphere Warmed?
Solar radiation transfers heat to Earth. The amount of solar radiation that reaches a
certain area is called insolation.
Higher latitudes receive less insolation due to a
greater angle of incidence. The angle of
incidence is the angle that occurs between a ray
reaching a surface and a line perpendicular to
that surface. It increases with latitude.
Very little solar radiation heats the atmosphere
directly. Solar radiation arrives in short
wavelengths, some of which pass through the
atmosphere to Earth’s surface, where they are
absorbed. Earth’s surface reradiates some of
this energy as longer, infrared waves. The atmosphere absorbs this infrared radiation and
convection transfers the thermal energy throughout the atmosphere.
Earth has a radiation budget that keeps incoming and outgoing energy in balance. Incoming
short-wave solar radiation is reflected and absorbed to various degrees. Albedo is the term
that describes the amount of radiation reflected by a surface. Forested regions and other
dark areas (low albedo), for example will absorb more radiation than areas covered in ice
and snow (high albedo).
What is atmospheric pressure?
Atmospheric pressure is the pressure exerted by the mass of air above any point on Earth’s
surface. Atmospheric pressure is measured with a barometer in Kilopascals (kPa). As the
atmosphere pressure changes, a capsule of flexible metal in an aneroid barometer expands
or contracts. Kilopascals measure the force per one square metre. Changes in atmospheric
pressure occur as a result of the following;
1.
Altitude: As altitude increases, atmospheric pressure decreases.
2. Temperature: Warm air is less dense than cold air, resulting in lower
atmospheric pressure.
3. Humidity: Humidity is a measurement that describes the amount of water vapour
in air. The greater the humidity, the lower the atmospheric pressure.
High Pressure System
Air cools and becomes more dense
Air mass contracts, draws in surrounding air,
and sinks
Due to weight of extra air, atmospheric
pressure increases; high pressure air moves
outward toward areas of low pressure,
creating wind.
Wind flows clockwise in the northern
hemisphere
Air becomes warmer and drier as it sinks,
bringing clear skies
Low Pressure System
Air warms and becomes less dense
Air mass expands and rises
Air pressure at Earth’s surface decreases
and draws in air from areas of high pressure,
creating wind.
Wind flows counterclockwise in the northern
hemisphere
Water vapour condenses as air cools,
bringing we weather.
What is Air Mass?
An air mass is a parcel of air with similar temperature and humidity throughout. Conditions
in an air mass become like Earth’s surface below it. When an air mass cools over a cold
region, a high pressure systems forms. Air masses that travel over warm regions may
develop into low pressure systems. The boundary between two air masses is called a front.
An approaching front means a change in weather. The extent of the change depends on the
amount of difference between conditions in the two air masses.
What is Weather?
Weather is the condition of the atmosphere in a specific place and at a specific time.
Weather describes all aspects of the atmosphere, including temperature, atmospheric
pressure, humidity, and wind speed and direction. Weather is closely connected to heat
transfer in the atmosphere. As heat is transferred, convection moves air and thermal
energy throughout the troposphere, causing various kinds of weather.
Several types of extreme weather occur on Earth, including thunderstorms, tornados, and
tropical cyclones.
A tornado is a violent funnel-shaped column of air. It is found when high altitude winds
meet large thunderstorms. Surface winds caused by tornadoes can reach 400 km/h.
Tropical cyclones, or hurricanes, result from the exchange of thermal energy in the tropics.
Warm moist air is lifted high into the atmosphere. As rain is produced, thermal energy is
released. Warm air rushes to replace the rising air, and the Coriolis effect forces the air
to rotate. The result is a massive, spinning storm.
How is Wind Generated on Earth?
Wind is the movement of air from an area of higher pressure to an area of lower pressure.
Geographic features such as mountains, oceans, and lakes greatly affect the characteristics
of local winds. Prevailing winds are winds that are typical fro a certain region. Over long
distances, wind is also affected by Earth’s rotation. The Coriolis effect is a change in the
direction of moving air, water, or objects due to Earth’s rotation. The Coriolis effect and
convection currents (rising warm air and sinking cool air) result in three major global wind
systems: the trade winds, the prevailing westerlies, and the polar easterlies.
Jet streams form in the upper troposphere due to convection currents and become bands of
fast-moving air in the stratosphere. They are so strong that airline pilots try to fly with
them.
Sci 10 – Unit 4(10.2)
Energy Transfer in the Atmosphere
Energy Transfer in the Atmosphere
Directions: READ pages 436-454 in your text book BC Science 10 (McGraw-Hill Ryerson 2008) and answer the following questions;
1. On a separate piece of paper, provide definitions for the following terms;
Atmosphere
Kilopascals (kPa)
Coriolis Effect
Albedo
Front
Barometer
Hurricanes
Prevailing Winds
2. On a separate piece of paper, answer the following questions using COMPLETE
SENTENCES;
a.
In your own words, describe how the Earth’s atmosphere formed and identify
the 2 elements that make up 99% of the atmosphere. (2 mks for quality of
response and inclusion of details)
b. In your own words, describe how the Sun transfers heat to the Earth and
explain what radiation budget means. (2 mks for quality of response and
inclusion of details)
c.
In your own words, describe what causes atmospheric pressure and identify 3
factors that can decrease atmospheric pressure. (2 mks for quality of response
and list of factors)
d. In your own words, describe how wind is formed and list three major global wind
systems and where they occur relative to the equator. (2 mks for quality of
response and list of systems)
3, Complete the table on the next page in order summarize the
characteristics of each of the layers in Earth’s atmosphere
You will be marked out of 10 for your ability to correctly and accurately
complete the table.
Total: ____ / 26
Complete the table below in order summarize the characteristics of each of
the layers in Earth’s atmosphere
You will be marked out of 10 for your ability to correctly and accurately
complete the table.
Layer
Altitude
above sea
level
Average
Temperature
Factors affecting composition
Troposphere
0-10 km
Stratosphere
The stratosphere contains the ozone layer
which absorbs much of the ultraviolet
radiation from the Sun which causes the
stratosphere to heat up
Mesosphere
Thermosphere
When charged particles in Earth’s
magnetic field collide with particles in the
thermosphere, the result is the aurora
borealis or “northern lights”.
Exosphere
This outer layer is not well defined and
merges with outer space.
300 -1700oC